Detection of solar-like oscillations in the bright red giant starsγPiscium andθ1 Tauri from a 190-day high-precision spectroscopic multi-site campaign

P. G. Beck; Eiji Kambe; M. Hillen; E. Corsaro; H. Van Winckel; E. Moravveji; J. De Ridder; S. Bloemen; S. Saesen; P. Mathias; P. Degroote; T. Kallinger; Tijl Verhoelst; Hiroyasu Ando; F. Carrier; B. Acke; R. Oreiro; A. Miglio; P. Eggenberger; Bun’ei Sato; K. Zwintz; P. I. Pápics; P. Marcos-Arenal; Sara Alejandra Sans Fuentes; V. S. Schmid; C. Waelkens; R. H. Østensen; J. M. Matthews; M. Yoshida; Hideyuki Izumiura; Hisashi Koyano; S. Nagayama; Yasuhiro Shimizu; N. Okada; Kiichi Okita; Akihiro Sakamoto; Tomoyasu Yamamuro; C. Aerts

doi:10.1051/0004-6361/201323019

Ask about this paper

Answers are grounded in this paper and cite their sources.

Abstract

Context. Red giants are evolved stars that exhibit solar-like oscillations. Although a multitude of stars have been observed with space telescopes, only a handful of red giant stars were targets of spectroscopic asteroseismic observing projects.

Discussion

No takes yet. Share an insight, caveat, or question.

Cite This Study

Beck et al. (2014) studied this question.

synapsesocial.com/papers/6a92e16871c7499eda18447f https://doi.org/10.1051/0004-6361/201323019

View Full Paper

Ask AI

Bookmark

Share

Detection of solar-like oscillations in the bright red giant starsγPiscium andθ1 Tauri from a 190-day high-precision spectroscopic multi-site campaign

Ask about this paper

Abstract

Discussion

Cite This Study

Detection of solar-like oscillations in the bright red giant starsγPiscium andθ1 Tauri from a 190-day high-precision spectroscopic multi-site campaign

Ask about this paper

Abstract

Discussion

Cite This Study

Keep reading

Keep reading